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A microscopic study of neutron stars’ structure
Published online by Cambridge University Press: 12 April 2016
Abstract
Starting from the nuclear interactions which are used to calculate the properties of atomic nuclei, we derive a new equation of state (EOS) for neutron star matter. With this realistic EOS, we calculate the structure of non-rotating neutron stars.
- Type
- Part 9. Population and Neutron Star Properties
- Information
- International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 657 - 658
- Copyright
- Copyright © Astronomical Society of the Pacific 2000